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Reading the Blueprints of Creation

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HOW TO SURVEY THE COSMOS IN FOUR NOT-SO-EASY STEPS<br />

THE SLOAN DIGITAL SKY SURVEY, <strong>the</strong> most advanced <strong>of</strong> <strong>the</strong> current generation <strong>of</strong> astronomical surveys, is compiling an atlas<br />

<strong>of</strong> a quarter <strong>of</strong> <strong>the</strong> sky. It will take five years, using a dedicated 2.5-meter telescope atop Apache Point in New Mexico.<br />

1<br />

2<br />

THE TELESCOPE operates in camera mode on clear nights, taking<br />

pictures through five color filters at <strong>the</strong> rate <strong>of</strong> 20 square degrees<br />

an hour—netting millions <strong>of</strong> celestial bodies per night.<br />

GALAXIES and o<strong>the</strong>r objects are identified by s<strong>of</strong>tware and<br />

selected for follow-up spectroscopy. The object shown here<br />

is <strong>the</strong> spiral galaxy UGC 03214 in <strong>the</strong> constellation Orion.<br />

3 1.0 4<br />

0.8<br />

Relative Flux<br />

0.6<br />

0.4<br />

0.2<br />

S D S S C O L L A B O R A T I O N<br />

OPTICAL FIBERS are plugged into a metal plate with 640 holes.<br />

Each fiber channels light from a celestial body to a spectrograph,<br />

which operates when <strong>the</strong> sky is not so clear.<br />

0<br />

400 600 800<br />

Wavelength (nanometers)<br />

THE SPECTRA THAT RESULT provide a precise way to classify<br />

objects. From <strong>the</strong>m, astronomers also determine <strong>the</strong><br />

redshifts, hence distances, <strong>of</strong> <strong>the</strong> objects.<br />

w w w . s c i a m . c o m S C I E N T I F I C A M E R I C A N 57<br />

COPYRIGHT 2004 SCIENTIFIC AMERICAN, INC.

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